PLANES

Unfolding the Evolution of Planetary Systems

 Coordinatore UNIVERSIDAD AUTONOMA DE MADRID 

 Organization address address: CALLE EINSTEIN, CIUDAD UNIV CANTOBLANCO RECTORADO 3
city: MADRID
postcode: 28049

contact info
Titolo: Ms.
Nome: Ana
Cognome: Amigo
Email: send email
Telefono: +34 91 4972897
Fax: +34 91 4972978

 Nazionalità Coordinatore Spain [ES]
 Totale costo 100˙000 €
 EC contributo 100˙000 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2010-RG
 Funding Scheme MC-IRG
 Anno di inizio 2010
 Periodo (anno-mese-giorno) 2010-09-01   -   2014-08-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    UNIVERSIDAD AUTONOMA DE MADRID

 Organization address address: CALLE EINSTEIN, CIUDAD UNIV CANTOBLANCO RECTORADO 3
city: MADRID
postcode: 28049

contact info
Titolo: Ms.
Nome: Ana
Cognome: Amigo
Email: send email
Telefono: +34 91 4972897
Fax: +34 91 4972978

ES (MADRID) coordinator 100˙000.00

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

evolution    dwarfs    stars    planet    sequence    evolved    envelope    sub    survival    mass    theoretical    planetary    planets    stellar   

 Obiettivo del progetto (Objective)

'Most of the exoplanets discovered to date orbit solar mass main-sequence stars. Essential to the detection and characterization of extrasolar planets is the knowledge of planetary systems around as many diverse stars as possible. In this context, surveys are now targeting planets around stars that have evolved off the Main Sequence, because, so far, it is one of the few means we have of directly determining the influence of the stellar mass on the planet formation mechanism.

With searches of planets around evolved pulsating B sub-dwarfs, red giant stars, and white dwarfs underway, it is paramount to advance theoretical research in how stellar evolution affects the architecture of planetary systems. With this project we aim to determine: (i) accurate orbital ranges where planets are expected to be found around evolved stars, (ii) the minimum masses for the survival of planets inside the stellar envelope of evolved stars, and (iii) the effects of sub-stellar objects on the common envelope evolution. The main goals of the program are to provide the theoretical framework to understand first how stellar evolution influences planet survival and second how planets affect the evolution of stars.'

Introduzione (Teaser)

To trace the origins of Earth and life in the Universe, EU-funded scientists studied planet formation and evolution, including the material around stars where planets form.

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